XENON1T solar axion and the Higgs boson emerging from the dark
Giacomo Cacciapaglia, Chengfeng Cai, Mads T.Frandsen, Martin, Rosenlyst, Hong Hao Zhang

TL;DR
This paper proposes a new dark matter production mechanism linking the Higgs boson and a light pseudo-scalar, explaining the XENON1T excess and predicting observable signals like gravitational waves and exotic decays.
Contribution
It introduces a composite dark sector model where a light pseudo-scalar explains the XENON1T excess and predicts testable phenomena in future experiments.
Findings
Pseudo-scalar produced in the sun explains XENON1T excess.
Dark Matter candidate has a mass around 50 TeV, beyond current detection.
Predicted gravitational waves and exotic decays are within future experimental reach.
Abstract
In a recent letter we proposed a new non-thermal mechanism of Dark Matter production based on vacuum misalignment, where both the Higgs boson and a very light pseudo-scalar emerge from the Dark sector. In this letter, we identify the parameter space in a composite scenario where the light pseudo-scalar can be produced in the sun and explain the XENON1T excess in electron recoil data. The model's Dark Matter candidate has a mass around TeV and out of range for Direct Detection. Testable predictions include Gravitational waves at frequencies in the Hz range from a cosmological phase transition, an exotic decay with rates testable at a future Tera-Z collider, and an enhancement by % of the branching ratio , not enough to explain the KOTO anomaly. All these predictions may be…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
